UBC 327

0.13 UTI

0.77

C_N

0.94

C_dens

1.0

C_C3

0.0

C_lit

0.23

C_dup

N_m (P>50%) 141

Core radius and density 1.5 [pc], 4.7 [pc^-2]

C3 classification AA

C_N 0.77 Rich
C_dens 0.94 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.23 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

ℹ️

UBC 327 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 6 years.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for UBC 327 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	251.751	-25.807	0.601	2.709	-2.669	22.025
Castro-Ginard et al.	2020	251.739	-25.799	0.574	2.751	-2.654	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	B_frac	BSS
UCC	99999–	1.55	2.2	–	977	–	–	–	–
Kounkel et al.	2020	1.55	2.20	–	977	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
ESO 518 03	76.6	251.75	-25.8	0.59	2.72	-2.67	22.02	0.74

💡 Note: The % column shows the percentage of members that UBC 327 shares with each listed object.

Visualization

ℹ️